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This shows you the differences between two versions of the page.

--- gc5_program [2019/09/09 17:21] – [Tuesday: Salle des séminaires Evry Schatzman (basement)] gmamon
+++ gc5_program [2022/10/24 11:57] (current) – external edit 127.0.0.1
@@ Line 13: / Line 13: @@
 |11:30| //Justin Read//| Dark matter heats up in dwarf galaxies|
 |11:50| //Khyati Malhan//| Understanding the origin and morphology of the stellar streams as revealed by Gaia DR2|
-|12:10| //Nathaniel Starkman//| Extending the Pal5 Stream Detection Limits & Using Manifold Learning Techniques to Identify Stream Progenitors|
-|12:30| //Jason Sanders//| Measuring the Milky Way bar’s pattern speed using proper motion data and full 6D data|
 |12:50| |LUNCH|
 |14:45| | Analysis of mocks|
@@ Line 22: / Line 20: @@
 ===== Tuesday: Salle des séminaires Evry Schatzman (basement) =====
 ^Time^Speaker^Topic^
-|9:30 | | |
+|9:30| //Nathaniel Starkman//| Extending the Pal5 Stream Detection Limits & Using Manifold Learning Techniques to Identify Stream Progenitors|
-|10:30 |//Simon Rozier//|Linear stability of stellar rotating spheres|
+|9:50| //Jason Sanders//| Measuring the Milky Way bar’s pattern speed using proper motion data and full 6D data|
+|10:10 |//Simon Rozier//|Linear stability of stellar rotating spheres|
 |11:00| |COFFEE BREAK (Entrance Hall)|
-|11:30 |//Tadeja Versic//|Observational requirements to resolve the core-cusp problem|
+|11:20 |//Tadeja Versic//|Observational requirements to resolve the core-cusp problem|
-|11:50 |//Antonio Sollima//|Detection of the tidal tails of Galactic globular clusters using 5D mixture modelling|
+|11:40 |//Antonio Sollima//|Detection of the tidal tails of Galactic globular clusters using 5D mixture modelling|
-|12:10| |Analysis of mocks|
+|12:00| |Analysis of mocks|
 |13:00| | LUNCH|
 |14:45| |Analysis of mocks|